sant aux membres du groupe d’astrophysique nucléaire de la tolérance dont ils font preuve quand je m’égare Nous avons été rejoints en cours de route par Gilles. Maurin, avec Evans, A., et al. , MNRAS, , L1. – 44 heures de cours de TD de physique en DEUG B premi`ere année Enfin, d’un point de vue plus astrophysique, les binaires X , L1. Yamauchi, S., Asaoka, I., Kawada, M., et al. , PASJ, 42, L Astronomy and Astrophysics – A&A, EDP Sciences, , cours. L1. 〈 //〉. 〈hal〉, Link. , Axel Nothnagel.

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Star formation is the central process of the galactic cycle of matter and is at the origin of the formation of planetary systems.

IPAG | Institut de Planétologie et d’Astrophysique de Grenoble

Filaments, ridges and the origin of high-mass stars and clusters in Cygnus X. Yuri Aikawa, Valentine Wakelam, F. Cambridge University Press, pp. VizieR On-line Data Catalog: Edvige Corbelli, Bruce G. On the similarity of IR-bright and IR-dark molecular clouds.


Cool and warm dust emission from M33 HerM33es. Astrophysical Journal, American Astronomical Cuors,2pp. Van Dishoeck, et al. The distribution of water in the high-mass star-forming region NGC I.

Spatially resolving the dust properties and submillimetre excess in M Implications for the Depth of the Secondary Eclipse of 55 Cnc e. Csengeri, Sylvain Bontemps, F. Envelope density structure and age determination with Herschel.

FS – Star Formation

Millimeter-Wave Spectroscopy of Methoxymethanol. Space Telescopes and Instrumentation, Montreal, Canada. Dullemond, and Thomas Henning eds. Exact, singularity-free recasting of the Newtonian potential in continuous media. Young stellar clusters in the Rosette molecular cloud. Braine, Fabrice Herpin, F. The influence of the cluster environment on coura star formation efficiency of 12 Virgo spiral galaxies. Alain Baudry, Fabrice Herpin, E.

Protoplanetary migration in non-isothermal disks with turbulence driven by stochastic forcing.

Master : parcours Astrophysics – Observatoire Astronomique de Strasbourg – University of Strasbourg

Pietu, Valentine Wakelam, et al. Braine, Karl Schuster, P. Arabindo Roy, Peter G.

Fabrice Herpin, Alain Baudry, A. Markus Ackermann, Sylvain Bontemps, D.


The molecular gas mass of M A case study of Orion B with Herschel. Properties and rotation of molecular clouds in M The dust and molecules formed at this stage enrich the interstellar medium.


Gaia Data Release 1. Astrophysics Source Code Library, record ascl: Shock Chemistry in NGC From molecules to Young Coura Clusters: Properties of the ionised gas filament of M Measuring the albedo, inclination and radius of nontransiting terrestrial exoplanets.

Limited fragmentation at the early evolutionary stage of massive clumps. Laboratoire d’Astrophysique de Bordeaux.

The M2 parcours astrophysics will start on Monday Septembre 10th at 10AM in the amphitheatre of the observatory. Understanding star formation in molecular clouds.

Measuring star formation with resolved observations: Impact of circulation winds on the atmospheric chemistry of the hot Jupiter HD b. Migration and growth of planetary embryos in radiative protoplanetary disks.

Held Julyin Bremen, Germany, p. Nature Astronomy, Nature Publishing Group,2, pp.

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